Search Publications

Low-energy particle oscillations and correlations with hydromagnetic waves in the Jovian magnetosphere: Ulysses measurements
DOI: 10.1029/96JA01296 Bibcode: 1996JGR...10117305K

Krupp, N.; Tsurutani, B. T.; Lanzerotti, L. J. +1 more

We report on measurements of energetic particle modulations (ions and electrons with energies E>50 keV) observed by the heliosphere instrument for spectra, composition, and anisotropy at low energies (HI-SCALE) aboard the Ulysses spacecraft that were associated with the only hydromagnetic (HM) wave event measured inside the Jovian magnetosphere…

1996 Journal of Geophysical Research
Ulysses 4
A paradigm revisited: the accretion disc in AGNs and quasars
DOI: 10.1093/mnras/282.1.117 Bibcode: 1996MNRAS.282..117G

Gondhalekar, P. M.; Kellett, B. J.; Rouillon-Foley, C.

A statistical comparison of model spectra of a thin bare accretion disc plus power-law and observations of over 400 active galactic nuclei (AGNs) and quasars are presented. This comparison is not limited to the optical/ultraviolet region of the observed spectra, as has often been the case in the past, but is extended over the entire ~4 eV to ~2 ke…

1996 Monthly Notices of the Royal Astronomical Society
IUE 4
The Weak Blue Bump of H2106-099 and Active Galactic Nuclei Dereddening
DOI: 10.1086/176722 Bibcode: 1996ApJ...457..199G

Ohashi, T.; Sakao, T.; Remillard, R. A. +3 more

We present multifrequency spectra of the Seyfert 1 galaxy H2106-099, from radio to hard X-rays, spanning over a decade of observations. The hard X-ray (2-20 keV) spectrum measured with Ginga was not unusual, with a log slope (Fυ ∝ Eα), of -0.80±0.02 on 1988 May 18 and -1.02±0.10 on 1988 May 22/23 UT, and with no significant o…

1996 The Astrophysical Journal
IUE 4
Recurrent variations of anomalous oxygen in association with a corotating interaction region
DOI: 10.1007/s00585-996-0585-6 Bibcode: 1996AnGeo..14..585R

Fränz, M.; Keppler, E.; Reuss, M. K.

The fluxes of anomalous oxygen (E ranging from 3.5-6.8 MeV/amu), as measured by the EPAC instrument on ULYSSES, show a recurrent variation with the solar rotation period, which is anticorrelated with the fluxes of particles accelerated at the shocks of a corotating interaction region (CIR), and correlated with the fluxes of galactic cosmic rays kn…

1996 Annales Geophysicae
Ulysses 4
Voyager Observations of the Companiion of the Classical Cepheid S MUSCAE
DOI: 10.1086/118009 Bibcode: 1996AJ....112..264E

Evans, Nancy Remage; Holberg, J. B.; Polidan, Ronalds S.

We have observed the companion of the Cepheid S Mus with the Voyager ultraviolet spectrometer, including a spectrum of the background. We have derived the energy distribution from 912 to 3200 Å using the reddening obtained from Cepheid colors corrected for the effect of the companion. This has been compared with three Morgan-Keenan "dagger" spectr…

1996 The Astronomical Journal
IUE 4
Classification of ultraviolet stellar spectra using artificial neural networks
Bibcode: 1996BASI...24...21G

Gulati, R. K.; Gupta, Ranjan; Gothoskar, Pradeep +1 more

Scheme based on the artificial neural networks (ANNs) trained with multi-layer back propagation using single level network for classifying ultraviolet spectra in the IUE Low-Dispersion Spectra Reference Atlas is presented. We compare the classification results obtained from single-level network with the one from multi-level neural tree network. Bo…

1996 Bulletin of the Astronomical Society of India
IUE 4
ULYSSES observations of double ion beams associated with coronal mass ejections
DOI: 10.1016/0273-1177(95)00589-7 Bibcode: 1996AdSpR..17d.303H

Balogh, A.; Phillips, J. L.; Feldman, W. C. +1 more

Coronal mass ejections (CME's) are thought to result from the loss of stability within a magnetically confined coronal structure leading to its radial expansion into interplanetary space. As the CME expands into the corona current sheets will form between the expanding CME and surrounding field lines in the ambient wind. This configuration may lea…

1996 Advances in Space Research
Ulysses 3
Recent observations of the WR central star of the planetary nebula LMC-N66
DOI: 10.1007/BF00645491 Bibcode: 1996Ap&SS.238...55P

Peña, Miriam; Maza, Jose; Peimbert, Manuel +2 more

The recent evolution of the central star of the planetary nebula LMC-N66 is presented. Before 1987, it showed a weak continuum with aTeff≥120 000 K andLbol≈25 000L and in a few years it developed strong WR features (P Cygni line profiles in N v at 124.0 nm and C IV at 155.0 nm, wide HeII emission, etc.) typical of…

1996 Astrophysics and Space Science
IUE 3
A `Ulysses' Cosmic-Ray Latitude Gradient Observation and Modulation Models
DOI: 10.1007/BF00148010 Bibcode: 1996SoPh..163..397Q

Keppler, E.; Quenby, J. J.; Drolias, B. +2 more

The `EPAC' instrument on Ulysses is sensitive to relativistic cosmic rays when far from Jupiter and in the absence of energetic solar particles. Measurement of the latitude gradient of these particles, after correction for time variations, has been made for the 1993-1994 south polar pass. The average magnitude of the gradient is about the same or …

1996 Solar Physics
Ulysses 3
Astrometric positions of stars associated with nebulosities in the southern hemisphere.
Bibcode: 1996A&AS..115..517R

Rousseau, J. M.; Perie, J. P.

Several stars associated with nebulosities and cited by S. van den Bergh and W. Herbst are included in the preliminary programme for the HIPPARCOS mission. When performing preparatory measurements of plates, we encountered difficulties in identifying certain of these objects when relying only on coordinates, which led us to take advantage of this …

1996 Astronomy and Astrophysics Supplement Series
Hipparcos 3